Sulphur-rich cold gas around the hot core precursor G328.2551-0.5321 - An APEX unbiased spectral survey of the 2 mm, 1.2 mm, and 0.8 mm atmospheric windows

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Fig. 14

Abundance ratios of OCS and H₂S relative to SO₂ for each source for the layers at Τ = 100 Κ for G328.2551-0.5321 and the sample from Herpin et al. (2009) ordered according to their assumed age sequence, G328.2551-0.5321 being the youngest and IRAS 18162-2048 the most evolved.

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